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Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties

, , , , , , , , and . (2017)cite arxiv:1708.07842Comment: 34 pages including Appendix, 18 figures (4 in Appendix), 5 tables (1 in Appendix). Accepted for publication in ApJ.

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Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844 - 7.213: Lyman Alpha Demography of z ~ 7 Galaxies, , , , , , , , , and 3 other author(s). (2011)cite arxiv:1107.3159Comment: 14 pages, 8 figures, submitted to ApJ.A Turnover in the Galaxy Main Sequence of Star Formation at $M_* \sim 10^10 M_ødot$ for Redshifts $z < 1.3$, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1501.01080Comment: 16 pages, 7 figures. Accepted for publication in ApJ.Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties, , , , , , , , and . (2017)cite arxiv:1708.07842Comment: 34 pages including Appendix, 18 figures (4 in Appendix), 5 tables (1 in Appendix). Accepted for publication in ApJ.The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, , , , , , , , , and 54 other author(s). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, , , , , , , , , and 96 other author(s). (2011)cite arxiv:1105.3753.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics, , , , , , , , , and 112 other author(s). (2011)cite arxiv:1105.3754 Comment: 36 pages, 22 figures.Dust Properties of CII Detected z $\sim$ 5.5 Galaxies: New HST/WFC3 Near-IR Observations, , , , , , , , , and . (2017)cite arxiv:1707.02980Comment: 9 pages, 3 figures, 1 table. Accepted for publication in The Astrophysical Journal.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , and 49 other author(s). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST, , , , , , , , , and 57 other author(s). (2022)cite arxiv:2211.05792Comment: 41 pages, 20 figures, 6 tables, submitted to ApJL. Key results in Figures 13-15, discussed in Sections 7 and 8.CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2, , , , , , , , , and 28 other author(s). (2011)cite arxiv:1109.2588 Comment: 10 Pages, 5 Figures, Revised draft submitted to ApJ.